End-to-end validation process for the INTA-Nanosat-1B Attitude Control System

This paper describes the end-to-end validation process for the Attitude Control Subsystem (ACS) of the satellite INTA-NanoSat-1B (NS-1B). This satellite was launched on July 2009 and it has been fully operative since then. The development of its ACS modules required an exhaustive integration and a system-level validation program. Some of the tests were centred on the validation of the drivers of sensors and actuators and were carried out over the flying model of the satellite. Others, more complex, constituted end-to-end tests where the concurrency of modules, the real-time control requirements and even the well-formedness of the telemetry data were verified. This work presents an incremental and highly automatised way for performing the ACS validation program based on two development suites and an end-to-end validation environment. The validation environment combines a Flat Satellite (FlatSat) configuration and a real-time emulator working in closed-loop. The FlatSat is built using the NS-1B Qualification Model (QM) hardware and it can run a complete version of the on-board software with the ACS modules fully integrated. The real-time emulator, running on an industrial PC, samples the actuation signals and emulates the sensors signals to close the control loop with the FlatSat. This validation environment constitutes a low-cost alternative to the classical three axes tilt table, with the advantage of being easily configured for working under specific orbit conditions, in accordance with any of the selected tests. The approach has been successfully applied to the NS-1B in order to verify different ACS modes under multiple orbit scenarios, providing an exhaustive coverage and reducing the risk of eventual errors during the satellite's lifetime. The strategy was applied also during the validation of the maintenance and reconfiguration procedures required once the satellite was launched. This paper describes in detail the complete ACS validation process that was performed and it shows the most relevant errors detected and fixed during testing. Finally it summarises some of the most significant conclusions.     

以主轴系统刚度与总功耗之比值为目标函数的液体静压轴承优化设计方法

本文介绍以主轴系统刚度与总功耗之比值最大比值最大为目标函数、主轴系统刚度的校验准则为主要约束条件的液体静压轴承优化设计方法，与普通设计方法相比，两种不同结构液体静压承经优化设计后，其单位总功耗的主轴系统刚度都成倍增加。     

Solar Nebula Magnetohydrodynamics

The dynamical state of the solar nebula depends critically upon whether or not the gas is magnetically coupled. The presence of a subthermal field will cause laminar flow to break down into turbulence. Magnetic coupling, in turn, depends upon the ionization fraction of the gas. The inner most region of the nebula (≲0.1 AU) is magnetically well-coupled, as is the outermost region (≳10 AU). The magnetic status of intermediate scales (∼1 AU) is less certain. It is plausible that there is a zone adjacent to the inner disk in which turbulent heating self-consistently maintains the requisite ionization levels. But the region adjacent to the active outer disk is likely to be magnetically ``dead.' Hall currents play a significant role in nebular magnetohydrodynamics. Though still occasionally argued in the literature, there is simply no evidence to support the once standard claim that differential rotation in a Keplerian disk is prone to break down into shear turbulence by nonlinear instabilities. There is abundant evidence—numerical, experimental, and analytic—in support of the stabilizing role of Coriolis forces. Hydrodynamical turbulence is almost certainly not a source of enhanced turbulence in the solar nebula, or in any other astrophysical accretion disk. This revised version was published online in June 2006 with corrections to the Cover Date.     

机载雷达综合显示器的仿真实现

雷达综合显示器是一种能够灵活地把雷达一次信息、二次信息、地图背景和各种表格数据综合在同一个显示界面进行显示的雷达终端系统,可以形象地提供雷达威力范围内比较全面的综合信息。本文对应用Visual C＋＋程序设计来实现航空机载雷达综合显示器的仿真问题进行了探讨。     

导航星座自主导航技术--自主星历更新

自主星历更新是导航星座自主导航的关键技术之一,包括卫星轨道精密确定和轨道短时预报两个方面的内容。本文在系统地论述导航星座自主导航的信息处理流程的基础上,重点提出星座卫星轨道精密确定的自适应Kalman滤波算法。系统仿真结果表明：通过星间双向测量数据的滤波处理,能够获得高精度的卫星星历和较小的用户测距误差（URE）,满足高精度导航定位需求,初步证明导航星座自主导航信息处理流程及其星历更新算法的合理性和可行性。     

基于GIS的军事通信网络传输资源信息管理系统

依据工作中的实践和经验,结合现代技术的发展和成果,在信息系统分析与设计的基础上引入GIS技术,分析了管理信息系统与地理信息系统结合的优势,提出并设计了基于地理信息系统的军事通信网络传榆资源信息管理系统,对具有空间属性特征信息管理系统的设计和开发具有一定的借鉴和参考价值。     

星载跟踪控制系统设计及其抗扰动分析

针对星载目标跟踪要求高精度及快速响应能力,但同时存在力矩扰动等影响,分析提出了跟踪控制系统性能指标,根据预设指标,对系统进行了初步设计及串联滞后校正,并在增加加速度计的情况下,对系统进行了抗扰动分析.利用Matlab进行系统幅频特性仿真结果表明,设计的系统能较好满足预设指标,具有良好的稳定跟踪性能.     

无线电掩星技术在大气探测的应用

通过介绍GPS在大气探测中的应用,引入了一种新的研究大气模型的方法——无线电掩星技术。阐明了无线电掩星技术的发展历程、反演原理及应用前景,并结合我国航天实际,提出了一种利用北斗导航系统进行大气参数反演,修正航天器轨道测量数据,从而提高定轨精度的新思路。     

基于存储测试技术的强冲击波测量系统的设计与应用

针对有线式测量系统在弹药静爆威力试验中存在的问题,提出了一种基于存储测试技术的解决方案,描述了按照该方案研制的强冲击波测量系统的系统组成、结构和工作原理,并结合弹药静爆试验证明了该方案的可行性。     

有限推力轨迹优化问题的直接打靶法研究

研究了求解有限推力轨迹优化问题的直接打靶方法。说明了利用直接打靶法将最优轨迹问题转化为参数优化问题的基本转换方法 ;给出了状态和控制变量的等式 (或不等式 )约束的转化方法 ;从插值和数值积分两个方面对转换过程中产生的误差进行了深入分析。最后 ,以最优交会问题为例 ,说明了不同节点数目和积分步数对计算结果的影响